If θ and δ be the latitude of an observer and declination of a heavenly body respectively, the upper culmination of the body will be south of zenith if its zenith distance, is

1.

If θ and δ be the latitude of an observer and declination of a heavenly body respectively, the upper culmination of the body will be south of zenith if its zenith distance, is

[A].	δ - θ
[B].	θ - δ
[C].	θ + δ
[D].	(θ - δ)

Answer: Option B

Explanation:

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